Published September 1987 | Version v1
Journal article Metadata-only

γ radiation expected from the supernova 1987A in the Large Magellanic Cloud

Creators

  • 1. Moskovskij Inzhenerno-Fizicheskij Inst. (USSR)
  • 2. Gosudarstvennyj Komitet po Ispol'zovaniyu Atomnoj Ehnergii SSSR, Moscow. Inst. Teoreticheskoj i Ehksperimental'noj Fiziki
  • 3. Moskovskij Gosudarstvennyj Univ. (USSR). Gosudarstvennyj Astronomicheskij Inst. ''GAISh''

Description

Results of Monte-Carlo Simulations of expected photon spectra in the range 0.1-3.5 MeV emerging from SN 1987 A which are born either in the 56Co decay or by the young pulsar are presented. The influence of the variations of the parameters of expanding envelope on the results is demonstrated

Additional details

Additional titles

Original title (Russian)
γ-излучение, ожидаемое от сверхновой 1987A в Большом Магеллановом Облаке

Publishing Information

Journal Title
Pis'ma Astron. Zh.
Journal Volume
13
Journal Issue
9
Series
Pis'ma Astron. Zh.
Journal Page Range
744-750
ISSN
0320-0108
CODEN
PAZHD

INIS

Country of Publication
Russian Federation
Country of Input or Organization
USSR
INIS RN
19038547
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
COBALT 56; FLUX DENSITY; GAMMA DECAY; GAMMA RADIATION; GAMMA SPECTRA; KEV RANGE 100-1000; MEV RANGE 01-10; PULSARS; STAR MODELS; STELLAR RADIATION; SUPERNOVAE
Descriptors DEC
BETA DECAY RADIOISOTOPES; BETA-PLUS DECAY RADIOISOTOPES; BINARY STARS; COBALT ISOTOPES; COSMIC RADIO SOURCES; DAYS LIVING RADIOISOTOPES; DECAY; ELECTROMAGNETIC RADIATION; ELECTRON CAPTURE RADIOISOTOPES; ENERGY RANGE; ERUPTIVE VARIABLE STARS; INTERMEDIATE MASS NUCLEI; IONIZING RADIATIONS; ISOTOPES; KEV RANGE; MATHEMATICAL MODELS; MEV RANGE; NUCLEAR DECAY; NUCLEI; ODD-ODD NUCLEI; RADIATIONS; RADIOISOTOPES; SPECTRA; STARS; VARIABLE STARS